1 #include "erfa.h"
2 
eraPnm06a(double date1,double date2,double rnpb[3][3])3 void eraPnm06a(double date1, double date2, double rnpb[3][3])
4 /*
5 **  - - - - - - - - - -
6 **   e r a P n m 0 6 a
7 **  - - - - - - - - - -
8 **
9 **  Form the matrix of precession-nutation for a given date (including
10 **  frame bias), IAU 2006 precession and IAU 2000A nutation models.
11 **
12 **  Given:
13 **     date1,date2 double       TT as a 2-part Julian Date (Note 1)
14 **
15 **  Returned:
16 **     rnpb        double[3][3] bias-precession-nutation matrix (Note 2)
17 **
18 **  Notes:
19 **
20 **  1) The TT date date1+date2 is a Julian Date, apportioned in any
21 **     convenient way between the two arguments.  For example,
22 **     JD(TT)=2450123.7 could be expressed in any of these ways,
23 **     among others:
24 **
25 **            date1          date2
26 **
27 **         2450123.7           0.0       (JD method)
28 **         2451545.0       -1421.3       (J2000 method)
29 **         2400000.5       50123.2       (MJD method)
30 **         2450123.5           0.2       (date & time method)
31 **
32 **     The JD method is the most natural and convenient to use in
33 **     cases where the loss of several decimal digits of resolution
34 **     is acceptable.  The J2000 method is best matched to the way
35 **     the argument is handled internally and will deliver the
36 **     optimum resolution.  The MJD method and the date & time methods
37 **     are both good compromises between resolution and convenience.
38 **
39 **  2) The matrix operates in the sense V(date) = rnpb * V(GCRS), where
40 **     the p-vector V(date) is with respect to the true equatorial triad
41 **     of date date1+date2 and the p-vector V(GCRS) is with respect to
42 **     the Geocentric Celestial Reference System (IAU, 2000).
43 **
44 **  Called:
45 **     eraPfw06     bias-precession F-W angles, IAU 2006
46 **     eraNut06a    nutation, IAU 2006/2000A
47 **     eraFw2m      F-W angles to r-matrix
48 **
49 **  Reference:
50 **
51 **     Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855.
52 **
53 **  Copyright (C) 2013-2014, NumFOCUS Foundation.
54 **  Derived, with permission, from the SOFA library.  See notes at end of file.
55 */
56 {
57    double gamb, phib, psib, epsa, dp, de;
58 
59 
60 /* Fukushima-Williams angles for frame bias and precession. */
61    eraPfw06(date1, date2, &gamb, &phib, &psib, &epsa);
62 
63 /* Nutation components. */
64    eraNut06a(date1, date2, &dp, &de);
65 
66 /* Equinox based nutation x precession x bias matrix. */
67    eraFw2m(gamb, phib, psib + dp, epsa + de, rnpb);
68 
69    return;
70 
71 }
72 /*----------------------------------------------------------------------
73 **
74 **
75 **  Copyright (C) 2013-2014, NumFOCUS Foundation.
76 **  All rights reserved.
77 **
78 **  This library is derived, with permission, from the International
79 **  Astronomical Union's "Standards of Fundamental Astronomy" library,
80 **  available from http://www.iausofa.org.
81 **
82 **  The ERFA version is intended to retain identical functionality to
83 **  the SOFA library, but made distinct through different function and
84 **  file names, as set out in the SOFA license conditions.  The SOFA
85 **  original has a role as a reference standard for the IAU and IERS,
86 **  and consequently redistribution is permitted only in its unaltered
87 **  state.  The ERFA version is not subject to this restriction and
88 **  therefore can be included in distributions which do not support the
89 **  concept of "read only" software.
90 **
91 **  Although the intent is to replicate the SOFA API (other than
92 **  replacement of prefix names) and results (with the exception of
93 **  bugs;  any that are discovered will be fixed), SOFA is not
94 **  responsible for any errors found in this version of the library.
95 **
96 **  If you wish to acknowledge the SOFA heritage, please acknowledge
97 **  that you are using a library derived from SOFA, rather than SOFA
98 **  itself.
99 **
100 **
101 **  TERMS AND CONDITIONS
102 **
103 **  Redistribution and use in source and binary forms, with or without
104 **  modification, are permitted provided that the following conditions
105 **  are met:
106 **
107 **  1 Redistributions of source code must retain the above copyright
108 **    notice, this list of conditions and the following disclaimer.
109 **
110 **  2 Redistributions in binary form must reproduce the above copyright
111 **    notice, this list of conditions and the following disclaimer in
112 **    the documentation and/or other materials provided with the
113 **    distribution.
114 **
115 **  3 Neither the name of the Standards Of Fundamental Astronomy Board,
116 **    the International Astronomical Union nor the names of its
117 **    contributors may be used to endorse or promote products derived
118 **    from this software without specific prior written permission.
119 **
120 **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
121 **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
122 **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
123 **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE
124 **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
125 **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
126 **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
127 **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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129 **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
130 **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
131 **  POSSIBILITY OF SUCH DAMAGE.
132 **
133 */
134